What the numbers refer to

A body with no sea level

On Earth the zero of height is found rather than chosen — water settles onto the equipotential surface by itself. Nowhere else has one, and the difference is measurable: Clairaut's theorem predicts the Earth's flattening from its own gravity field to twelve metres at the pole and misses Mars's by 2.2 kilometres.

Every height on Earth is measured from a surface that nobody had to choose. Water finds the equipotential surface by itself; mean sea level is a physical object; the geoid is a description of something that already exists, and the reference ellipsoid was then defined to be a level surface so that the geometrical datum and the physical one would agree.

That arrangement is so convenient that it is easy to mistake for the natural order of things. It is not available anywhere else. Mars has no sea, so the zero of Martian elevation is a decision, and it has been made twice this century: an atmospheric-pressure surface — the level at which the mean pressure equals the triple point of water — until 2001, and an equipotential surface tied to the mean equatorial radius since. Those are different surfaces. The elevation of a Martian place changed by kilometres without the ground moving.

What this site can compute, rather than cite, is the relation between a body’s shape and its gravity field, and how far each body is from having them agree.

Shape predicted from field, against shape as published. Clairaut's theorem gives a body's flattening from two numbers of its gravity field: J₂, which is how its mass is arranged, and m = ω²a³/GM, which is how fast it spins. For a body in hydrostatic equilibrium the prediction is the shape, and the diagonal is where such a body sits. Earth is on it to 0.05 per cent — 12 metres at the pole, out of twenty-one kilometres of flattening. Mars is 12.5 per cent off it, which is 2.23 kilometres, and the excess is Tharsis: a body carrying a continent-sized volcanic load is not a fluid figure, so its ellipsoid is not one of its own level surfaces, and its zero of height has to be chosen rather than found.
Fig. 1 Each body’s flattening as its own gravity field predicts it, against the flattening its published radii have. Clairaut’s theorem gives the first from J₂, which says how the mass is arranged, and m = ω²a³/GM, which says how fast the body spins. A body in hydrostatic equilibrium sits on the diagonal. The Earth is on it to 0.05 per cent — twelve metres at the pole out of twenty-one kilometres of flattening — and Mars is 12.5 per cent off it, which is 2.23 kilometres.

Clairaut’s theorem as a prediction rather than a check

The site already carries Clairaut’s theorem in its terrestrial form, where it relates the geometrical flattening to the gravity flattening and is used to audit the normal field: the ellipsoid is a level surface shows the two summing to 5m/2 with a residual that is second order in f, which is what a first-order theorem is entitled to be wrong by.

Turned round, the same theorem is a prediction:

f32J2+m2,m=ω2a3GMf \approx \tfrac{3}{2}J_2 + \tfrac{m}{2}, \qquad m = \frac{\omega^2 a^3}{GM}

with J₂ the dynamical form factor and m the ratio of centrifugal to gravitational acceleration at the equator. Both inputs are properties of the field, and the output is a property of the shape. For a body in hydrostatic equilibrium — a fluid figure, settled — the prediction is the shape.

Clairaut's theorem, and the term it drops. Clairaut's theorem says the flattening of a rotating body plus the flattening of the gravity on it equals five halves of the ratio of centrifugal to gravitational acceleration at the equator. Measured on WGS84: f = 3.3528e-3, f* = 5.3024e-3, and their sum is 8.65525e-3 against the theorem's 8.62447e-3. The residual is 3.08e-5, which is 2.74 times f² — second order, which is what a first-order theorem is entitled to be wrong by.
Fig. 2 The terrestrial form of the same theorem, audited. The flattening of the figure plus the flattening of gravity equals five halves of m, with a residual of 3.1 × 10⁻⁵ that is 2.74 times f² — second order, which is exactly what a first-order theorem may be wrong by and is the reason the prediction below is quoted to two figures rather than five.

The Earth’s numbers: J₂ = 1.0826 × 10⁻³ and m = 3.4614 × 10⁻³, giving a predicted flattening of 1/298.10 against a published 1/298.26. The disagreement is 0.055 per cent, which is twelve metres at the pole.

Twelve metres is small enough to be second-order theory and nothing else. The Earth is a fluid figure to the accuracy a first-order theorem can see.

Mars is not

Mars’s numbers: J₂ = 1.9554 × 10⁻³, m = 4.5953 × 10⁻³, predicted flattening 1/191.2. Its published radii give 1/169.9. The prediction is out by 12.5 per cent, which at the pole is 2.23 kilometres.

That is not a failure of the theorem and it is not a bad measurement. It is the finding: Mars is not in hydrostatic equilibrium, because it carries Tharsis — a volcanic province the size of a continent and several kilometres high, with a corresponding mass excess that the rest of the body has not relaxed away. A body carrying a load like that has a figure its own spin cannot explain, and its reference ellipsoid is therefore not one of its level surfaces.

Every consequence a coordinate system has follows from that one sentence.

How far apart a body's two candidate zero surfaces are. The gap at the pole between the ellipsoid a body's coordinates are published on and the level surface its own gravity field would settle into. On Earth it is 12 metres, because the reference ellipsoid was defined to be a level ellipsoid — the sea had already found the answer and the definition followed it. On Mars it is 2.23 kilometres. That is the size of the convention: an elevation on a body with no sea is a statement about which surface was meant, and Mars has used two different ones this century — an equipotential surface, chosen in 2001; an atmospheric-pressure surface before that.
Fig. 3 The gap at the pole between the ellipsoid a body’s coordinates are published on and the level surface its own gravity field would settle into. On Earth it is twelve metres, because the reference ellipsoid was defined to be a level ellipsoid — the sea had already found the answer and the definition followed it. On Mars it is 2.23 kilometres, and on the Moon, whose coordinates use a sphere by convention, 536 metres.

A second route to the same conclusion

The site’s normal-field machinery takes four constants — a, f, GM and ω — and derives everything else in closed form, including J₂ itself. It was written for the Earth and nothing in it is about the Earth, which is a claim worth testing by handing it a planet.

Given Mars’s radii and its GM and rotation rate, the machinery returns J₂ = 2.392 × 10⁻³. The observed J₂ is 1.955 × 10⁻³. The derivation is 22 per cent high, and the reason is the same one: it computes the field of the level ellipsoid that has Mars’s shape, and Mars’s shape is not a level surface, so the field it would have if it were is not the field it has.

Two independent routes, one from shape to field and one from field to shape, disagreeing by the same fraction in opposite directions. That is the site’s usual standard of evidence, applied to a claim about a planet rather than about a projection.

The reason to trust the machinery when it is pointed at Mars is that it can be checked where checking is possible. On the Earth the same four constants reproduce the published equatorial and polar gravity, the published J₂ and the published polar radius to ten significant figures, none of which are inputs.

Every published constant, recomputed. The relative difference between each published WGS84 constant and the value derived here from the four that define the system — a, f, GM and ω. The largest gap is 1.2e-11, which is the last digit each constant is published to. Polar radius, equatorial and polar gravity, the dynamical form factor J₂ and the potential of the ellipsoid are all consequences of the definition rather than separate measurements.
Fig. 4 The normal field’s derived constants against the published ones, for WGS84. Equatorial gravity, polar gravity, J₂, the potential of the ellipsoid and the polar semi-axis are all computed from a, f, GM and ω, and all agree with the published values to the last digit those values carry. A derivation that reproduces five numbers it was not given is a derivation that can be pointed at a planet whose numbers nobody has published.

The distinction matters because a reader is entitled to ask what a 12.5 per cent disagreement on Mars is evidence of. It is not evidence about the arithmetic, which is exact and audited; it is not evidence about the constants, which are published to more digits than the comparison uses; and it is not evidence about the theorem, which the Earth’s case shows holding to a part in two thousand at a comparable flattening. What is left is the body.

Normal gravity, derived from four constants. Gravity on the surface of the level ellipsoid, by Somigliana's closed form, for WGS84 and Mars. Nothing here is measured: a, f, GM and ω go in and the whole curve comes out, rising 5186 milligal — 0.53 per cent — from equator to pole. The two open marks are the published values of equatorial and polar gravity for WGS84, which the derivation reproduces to ten significant figures rather than borrowing.
Fig. 5 Normal gravity from equator to pole, on the Earth and on Mars, from Somigliana’s closed form. Nothing here is measured: four constants go in and the whole curve comes out. Martian surface gravity is 3.71 m s⁻² at the equator against the Earth’s 9.78, and its equator-to-pole rise is a slightly larger fraction, because Mars spins at nearly the same rate on a smaller body. The machinery does not know which planet it is being asked about, which is the point of the figure.

What a zero of height is, once it has to be chosen

Three candidate surfaces are available on any body, and on Earth they nearly coincide, which is why the choice has never had to be argued in public.

A sphere of stated radius. The Moon’s coordinates use one: 1,737.4 km, by convention. It is simple, it is exactly reproducible, and it is a surface no physical process would ever pick — the Moon’s own J₂ implies a level flattening of 1/3,241, which puts the level surface 536 metres below the sphere at the pole.

An ellipsoid fitted to the topography. This is the Martian ellipsoid, and it is what most planetary maps are drawn on. It is a least-squares fit to a shape model, which makes it a summary of the topography rather than a physical surface, and the 2.23 km gap above is the amount by which those two ideas differ on Mars.

Three surfaces, and the two heights between them. The ellipsoid, the geoid and the ground, with the two heights a coordinate can carry. Ellipsoidal height h is what a satellite fix returns and is measured from a surface defined by four constants. Orthometric height H is what a level and a staff measure and is referred to the geoid — the equipotential surface that best fits mean sea level. They differ by the separation N, drawn here as 45 metres because that is a stated input rather than a computed one: a geoid model is a data product with a truncation degree in it, and this site computes rather than downloads. The arithmetic h = H + N is exact whatever N is.
Fig. 6 The three surfaces on Earth, and the two heights between them: the ellipsoid, which is four constants; the geoid, which is where water settles; and the ground. A terrestrial height is referred to the middle one and a satellite fix to the first, and the separation between them is a data product. On a body with no sea the middle surface is missing from this picture, and the question this essay is about is what takes its place.

An equipotential surface. The physically meaningful one: the surface water would follow, if there were water. It needs a gravity field model, which is a data product exactly as a geoid model is, and it needs one further decision that the Earth’s case hides — which equipotential. On Earth the sea picks the value of the potential; on Mars a number has to be chosen, and the choice made in 2001 was the potential of the surface whose mean equatorial radius is 3,396.19 km.

A level surface 1000 metres up, from equator to pole. A quarter of a meridian, with the ellipsoid and one surface of constant potential drawn on it. The surface is 1000.0 metres above the ellipsoid at the equator and 994.7 at the pole: it converges by 5.28 metres, which is 5.28 parts per thousand — the gravity flattening f*, to within second-order terms. The separation is drawn 400× life size; the ellipsoid's own flattening is not exaggerated and is a quarter of a pixel at this scale.
Fig. 7 Why the choice is not free even after the family is fixed: level surfaces are not parallel to each other. The one drawn a kilometre above the ellipsoid at the equator is closer to the ellipsoid at the pole, because gravity is stronger there and the same energy difference buys less height. Choosing which equipotential is the zero therefore changes elevations by different amounts in different places, which is the reason a vertical datum is a surface and not an offset.

What was computed, and how

Two constants per body are citations and everything else is derived. GM, ω and J₂ are taken as published, in the same sense the IAU radii already are: astronomy-celestial-mechanics.com owns these bodies as observed objects, and nothing here computes an orbit, a mass or a rotation rate. What is computed is what those numbers imply for the surface a coordinate is measured from, which is this site’s question.

m is computed rather than quoted, as ω²a³/GM, and it is worth looking at on its own. On Earth the spin contributes 51.6 per cent of the predicted flattening and the mass arrangement 48.4 per cent; on Mars the spin contributes 43.9 per cent. The two mechanisms are comparable in size on both bodies, which is why a theory that dropped either would be useless.

The predicted flattening is a first-order expression and the comparison respects that. The theorem’s next term is of order f², which for Mars is 3 × 10⁻⁵ against a flattening of 5.9 × 10⁻³ — half a per cent of the answer, against a disagreement of 12.5 per cent. The Earth’s residual, measured in the audit above at 2.74 f², is the empirical version of that bound and is what makes the Martian excess twenty times too large to be truncation.

The gap is reported at the pole because that is where a difference in flattening is largest and because it is the number a mapping decision actually feels. At the equator the two surfaces agree by construction: both are fitted to the same equatorial radius.

The refusal is Venus. Its measured flattening is zero to the precision of the published radii, and its predicted one is 6.7 × 10⁻⁶ — 41 metres on a body 6,000 km across, which is a tenth of the thickness of the layer of rock a radar altimeter is even sensitive to. A test that reported a large disagreement there would be reporting its own noise, and the machinery’s not doing so is what licenses the Martian number.

Three kinds of disagreement, and only one of them is about the body

Running the prediction across every body the site carries a gravity field for gives five rows, and reading them as a single ranking of “how far from equilibrium” would be wrong in three different ways.

body predicted f published f polar gap spin’s share of the prediction
Earth 1/298.10 1/298.26 −12 m 51.6 %
Mars 1/191.2 1/169.9 +2,225 m 43.9 %
Jupiter 1/15.01 1/15.41 −126 km 66.9 %
Moon 1/3,241 0 −536 m 1.2 %
Venus 1/148,900 0 −41 m 0.5 %

Jupiter’s is the theorem’s. Its flattening is a fifteenth, the theorem is a series in the flattening, and 2.6 per cent is about what a dropped second-order term is worth at that size. Nothing in that row is evidence about Jupiter.

Mars’s is the body’s, and it is the only row where that is true. Its flattening is small enough that the truncation is worth half a per cent, so a 12.5 per cent excess is twenty times too large to be the theory, and the Earth’s row is the control that says so at a comparable flattening.

The Moon’s and Venus’s are the datum’s. Their published flattening is not a small number that disagrees with the prediction; it is exactly zero, because both bodies’ coordinates are referred to a sphere by convention. So the gap in those two rows is not a statement about how far the body is from equilibrium at all — it is the size of the convention, which is precisely what this essay set out to measure. A lunar coordinate is published on a surface that the Moon’s own gravity field puts 536 metres above the pole of the level figure, and nobody thinks the Moon is a sphere.

Those two rows also isolate the other half of Clairaut’s expression. On the Earth the spin contributes 51.6 per cent of the predicted flattening and the mass arrangement 48.4; on Jupiter the spin contributes two thirds. On the Moon it contributes 1.2 per cent and on Venus 0.5, because both turn slowly enough that the centrifugal term nearly vanishes — Venus’s day is longer than its year. Their predicted figures are therefore almost pure J₂: a shape implied by how the mass is arranged and not at all by how the body spins. For the Moon that prediction is known to be a fossil rather than a current equilibrium, which is one more reason its sphere has never been replaced.

Jupiter, and where the first-order theory stops

Jupiter’s flattening is 1/15.4, which is not small, and Clairaut’s first-order theorem is a series in exactly that quantity. The prediction comes out 2.6 per cent from the published figure — 126 kilometres — and almost all of that is the theorem’s truncation rather than the planet’s departure from equilibrium. Jupiter is a fluid figure; it is simply too flattened for one term.

That is worth stating rather than burying, because it is the boundary of the argument. The Martian number is evidence about Mars only because Mars’s flattening is small enough for the first-order theory to be trusted to a per cent, which the Earth’s case demonstrates directly. On a body flattened by a tenth the same comparison would prove nothing.

The same boundary shows up in a second, unrelated measurement, which is the reason to trust it as a boundary rather than as an artefact of this calculation. The error of applying spherical formulae to a body’s own latitudes follows a law of 2f radians, and it holds to a third of a per cent for Mercury, the Earth and Mars while departing by 3.3 and 5.1 per cent for Jupiter and Saturn. The same two bodies leave the regime each time, because a first-order statement is a first-order statement wherever it appears.

Where the model stops

No geoid, and no areoid. The gap computed here is between the published ellipsoid and the level ellipsoid of the same equatorial radius, both of which are analytic surfaces. The actual Martian equipotential surface departs from either by kilometres in places, and computing that needs a spherical-harmonic gravity model, which is a data product with a truncation degree in it — the citation this site declined in height above what and declines again here. What is computed is the size of the discrepancy that makes the choice necessary, not the shape of the surface eventually chosen.

The topography is not modelled. Saying that the excess flattening is Tharsis is an attribution, not a measurement: this site has not integrated the mass of Tharsis and shown that it accounts for 2.23 kilometres of polar radius. That calculation is done in the planetary geodesy literature and its inputs are a shape model and a gravity model, neither of which is available here on the site’s own terms.

Two of the five rows cannot be read as measurements of a body. The Moon’s and Venus’s published flattenings are zero because their coordinates are referred to a sphere, not because either body has been measured as spherical, and this site carries no independent shape model for either. So the gap quoted for them is the distance between a convention and a prediction, with the third quantity — the actual figure — absent. The Moon in particular is known from laser ranging to carry a figure its present rotation cannot explain, and nothing here measures it; the row says only how far the adopted sphere is from the surface the Moon’s own field would settle into, which is the question the essay asks and not the question of what shape the Moon is.

The polar gap is a difference between two analytic surfaces of the same equatorial radius, so it is zero at the equator by construction and largest at the pole, and it is not the error in anybody’s elevation. An elevation’s error depends on which surface the elevation was actually referred to, and on Mars that has changed once in the period this site’s sources cover.

A triaxial body has no version of this at all. Vesta and Phobos are far too small for hydrostatic equilibrium to be a useful idea and far too irregular for one equipotential to be a sensible datum. Their published coordinates use a fitted triaxial figure, and the previous rung is where the machinery for measuring on one lives.

Who found it, and when

Clairaut published Théorie de la figure de la Terre in 1743, and its central theorem was the first result to connect a measurement anybody could make — the variation of gravity with latitude — to a quantity nobody could see directly, the flattening of the Earth. It settled an argument that had run for fifty years between the Cassinis, who measured the Earth as prolate, and the Newtonians, who predicted it oblate.

Its planetary use is recent, and Mars is the case that forced it. Mariner 9 in 1971 showed the Tharsis rise; the gravity field that came with it showed a J₂ that did not match the figure, and the mismatch has been the standard evidence for a non-hydrostatic Mars ever since. The Mars Orbiter Laser Altimeter, from 1997, produced the topography that made the modern areoid definable at all, and the current convention dates from a working-group decision in 2001.

The Moon’s sphere is older and more pragmatic: it was fixed by convention before there was any way to do better, and it has been kept because changing a datum invalidates every published coordinate, which is the argument a published coordinate is a result makes about the terrestrial case.

Where the ladder goes next

This rung and the one before it exhaust what the site set out to say about bodies: what a coordinate on one means, and what the surface it is measured from is. Both essays lean on a quantity that has appeared in every field of this site and has never been examined as a variable — the curvature of the surface being mapped, which on a sphere is one number, on an ellipsoid a function of latitude, and on Vesta a function of two coordinates varying by a factor of nearly three.

The impossibility argument this site is built on was made on a sphere, where the curvature is constant. Whether it survives a surface where it is not is the next question, and the answer changes what how small is flat enough means.

Named alongside this one

Essays reaching for the same objects. Nobody chose these; they are what the concept index makes visible.

What links here

Every essay whose body links to this one.

The objects this essay names

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Clairaut theoremClosed formConventionDynamical form factorEquipotentialFlatteningGeodetic datumGeoidHydrostatic equilibriumPlanetary datumRealisationVertical datum